Now we have the necessary tools to investigate lensing effects due to supermassive black holes (SMBHs) at the center of the Milky Way and thirteen other galaxies. Our main aim is to compare the lensing predictions of GR with those of EQG. To do so we numerically solve equations (REF ), (REF ), (REF ), and (REF ), to respectively find their deflection angles, angular positions of their images, their magnifications, and their time delays. Although lensing due to Sgr A* in GR has been extensively investigated numerically [1]}, [2]}, [3]}, [4]}, we recalculate the GR results with greater precision
for the mass of Sgr A* \(M=5.94\times 10^9 \, {\rm m}\) , which is at a distance \(D=2.43\times 10^{20} \, {\rm m}\)  from Earth [5]}.
